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The Impact of Pollution on Stellar Evolution Models

  • Authors: Aaron Dotter and Brian Chaboyer

Dotter & Chaboyer 2003 The Astrophysical Journal 596 496.

  • Provider: AAS Journals

Caption: Fig. 2.

Top panel: CMD of the Hyades sample with the mean polluted isochrone (solid line) and LOWESS fit (dashed line) superposed. Bottom panel: Scatter plot in Δ﹩M_{V}﹩ of the Hyades sample about the LOWESS fit. Superimposed are the differences between the 2 σ isochrones and the mean isochrone (dashed line: +2 σ; dotted line: −2 σ).

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